Ultraviolet Radiation and the Photobiology of Earth's Early Oceans

During the Archean era (3.9–2.5 Ga ago) the earth was dominatedby an oceanic lithosphere. Thus, understanding how life aroseand persisted in the Archean oceans constitutes a majorchallenge in understanding early life on earth. Using aradiative transfer model of the late Archean oceans, thephotobiological environment of the photic zone and the surfacemicrolayer is explored at the time before the formation of a significant ozonecolumn. DNA damage rates might have been approximately threeorders of magnitude higher in the surface layer of the Archeanoceans than on the present-day oceans, but at 30 m depth,damage may have been similar to the surface of the present-dayoceans. However at this depth the risk of being transported to surface waters in the mixed layer was high. The mixed layer mayhave been inhabited by a low diversity UV-resistant biota. Butit could have been numerically abundant. Repair capabilitiessimilar to Deinococcus radiodurans would be sufficient tosurvive in the mixed layer. Diversity may have beengreater in the region below the mixed layer and above the lightcompensation point corresponding to today's `deep chlorophyllmaximum'. During much of the Archean the air-water interface wasprobably an uninhabitable extreme environment for neuston. Thehabitability of some regions of the photic zone is consistentwith the evidence embodied in the geologic record, whichsuggests an oxygenated upper layer in the Archean oceans. Duringthe early Proterozoic, as ozone concentrations increased to acolumn abundance above 1 × 10¹⁷ cm^-2, UV stresswould have been reduced and possibly a greater diversity oforganisms could have inhabited the mixed layer. However,nutrient upwelling from newly emergent continental crusts mayhave been more significant in increasing total planktonic abundance inthe open oceans and coastal regions than photobiologicalfactors. The phohobiological environment of the Archean oceanshas implications for the potential cross-transfer of life betweenother water bodies of the early Solar System, possibly on earlyMars or the water bodies of a wet, early Venus.     

Electron Paramagnetic Resonance Study of a Photosynthetic Microbial Mat and Comparison with Archean Cherts

Organic radicals in artificially carbonized biomass dominated by oxygenic and non-oxygenic photosynthetic bacteria, Microcoleus chthonoplastes-like and Chloroflexus-like bacteria respectively, were studied by Electron Paramagnetic Resonance (EPR) spectroscopy. The two bacteria species were sampled in mats from a hypersaline lake. They underwent accelerated ageing by cumulative thermal treatments to induce progressive carbonization of the biological material, mimicking the natural maturation of carbonaceous material of Archean age. For thermal treatments at temperatures higher than 620 °C, a drastic increase in the EPR linewidth is observed in the carbonaceous matter from oxygenic photosynthetic bacteria and not anoxygenic photosynthetic bacteria. This selective EPR linewidth broadening reflects the presence of a catalytic element inducing formation of radical aggregates, without affecting the molecular structure or the microstructure of the organic matter, as shown by Raman spectroscopy and Transmission Electron Microscopy. For comparison, we carried out an EPR study of organic radicals in silicified carbonaceous rocks (cherts) from various localities, of different ages (0.42 to 3.5 Gyr) and having undergone various degrees of metamorphism, i.e. various degrees of natural carbonization. EPR linewidth dispersion for the most primitive samples was quite significant, pointing to a selective dipolar broadening similar to that observed for carbonized bacteria. This surprising result merits further evaluation in the light of its potential use as a marker of past bacterial metabolisms, in particular oxygenic photosynthesis, in Archean cherts.     

Photosynthesis in the Archean Era

The earliest reductant for photosynthesis may have been H₂. The carbon isotope composition measured in graphite from the 3.8-Ga Isua Supercrustal Belt in Greenland is attributed to H₂-driven photosynthesis, rather than to oxygenic photosynthesis as there would have been no evolutionary pressure for oxygenic photosynthesis in the presence of H₂. Anoxygenic photosynthesis may also be responsible for the filamentous mats found in the 3.4-Ga Buck Reef Chert in South Africa. Another early reductant was probably H₂S. Eventually the supply of H₂ in the atmosphere was likely to have been attenuated by the production of CH₄ by methanogens, and the supply of H₂S was likely to have been restricted to special environments near volcanos. Evaporites, possible stromatolites, and possible microfossils found in the 3.5-Ga Warrawoona Megasequence in Australia are attributed to sulfur-driven photosynthesis. Proteobacteria and protocyanobacteria are assumed to have evolved to use ferrous iron as reductant sometime around 3.0 Ga or earlier. This type of photosynthesis could have produced banded iron formations similar to those produced by oxygenic photosynthesis. Microfossils, stromatolites, and chemical biomarkers in Australia and South Africa show that cyanobacteria containing chlorophyll a and carrying out oxygenic photosynthesis appeared by 2.8 Ga, but the oxygen level in the atmosphere did not begin to increase until about 2.3 Ga.     

Chlorophyll Photosynthetic Potential in Wheat Stands in Dry and Humid Years

Influence of climatic conditions (total precipitation and sunshine duration) on the dynamics of chlorophyll photosynthetic potential (CPSP) and its relation to productivity of crop stands was studied with long- and short-stalked cultivars of winter wheat (Triticum aestivum L.). The reduction of the total exposure time to solar photosynthetically active radiation by 100 h per growing season (humid year) was shown to decrease CPSP by a factor of 1.3 and 1.5 in long-stalked and short-stalked cultivars, respectively. The decrease was mainly related to the suppression of biomass production, one of the main constituents of photosynthetic potential. Retardation of growth processes was manifested in a twofold decrease in the shoot number per m² on average; furthermore, morphological stages were delayed during early development. Suppression of growth processes by the shortened sunshine time was not compensated for by a 30% increase in specific chlorophyll content (as distinct from shade leaves), the other component of CPSP. It was shown that growth conditions have an effect on the correlation coefficient between CPSP and productivity.     

Potential Increase in Photosynthetic Efficiency from the Redistribution of Solar Radiation in a Crop

The efficiency of the conversion of photosynthetically activeradiation by C₃ plants falls off with increasing intensity.Hypothesis: an increase in the productivity of direct solarenergy will be achieved if, by redistribution, it is interceptedat a more uniform and lower intensity by a greater proportionof the leaf area of a crop. A model is developed which usesestimates of the proportions of clear and overcast conditionsfrom site records of solar radiation to calculate the resultantphotosynthetic productivity. The amounts of diffuse light anddirect light are estimated for clear conditions. The model predictsthat redistributing direct solar radiation over twice the leafarea at half the intensity would give an increase of 22% inannual productivity. The model gives reasonable values for theproductivity reductions reported for two shading regimes. Tomato plants were grown for 21 d in three cabinets under regimesthat differed from each other only in the distribution of PARenergy over the daily photoperiod: (a) 103 W m^–2 for halfthe photoperiod followed by 13 W m^–2, (b) 13 W m^–2followed by 103 W m^–2 and (c) 58 W m^–2 for the wholephotoperiod. The dry matter increase of plants under the uniformregime was 33% greater than the average of those in the twoasymmetric regimes. It is suggested that, in protected cultivation, screens of partiallyreflective material could be used to redistribute solar radiationfrom leaves exposed to high intensities on to shaded leavesand so raise the photosynthetic efficiency. Assuming an absorptionof direct light by the screens of 0.10, the increase in productivityis estimated to be 17%. Key words: Photosynthesis, C₃, canopy, solar energy, solar redistribution, light interception, partial reflection, growth cabinet, glasshouse, tomato     

Localization of Chromosome Regions Controlling High Photosynthetic Potential in Russian Rice Cultivars

Breeding practice defined the main ways to increase crop yield: morphotype change, exploitation of heterosis, and increase in photosynthesis effectiveness. We identified donors and sources of high photosynthetic potential genetic system and polymorphic loci controlling photosynthetic efficiency in Russian rice cultivars. Thirty-two Russian rice cultivars were used as material. The content of chlorophyll a and b and carotenoids was measured at the beginning of tillering, heading, and flowering stages by a Genesys 8 spectrophotometer. Twenty plants of each cultivar in two replications were used for measurement. SSR markers were used. DNA was extracted by the STAB method. Polymerase chain reaction (PCR) and visualization of amplification products were performed under the International Rice Research Institute (IRRI) protocol. Donors of high contents of each pigment were found. A high level of polymorphism for the loci connected with photosynthesis effectiveness in Russian rice cultivars will allow us to create new cultivars with improved characters by hybridization. Six markers significantly divided cultivar groups with different photosynthetic rate, three of them (RM154, RM600, RM5508) were related to the content of carotenoids, two markers (RM347, RM240) were related to specific leaf weight (SLW) control, and two others (RM154, RM509) were related to the chlorophyll a content.     

Remote Assay for Chlorophyll Photosynthetic Potential of Crops on the Example of Wheat

An optical remote assay for biological production of crops in the field during the vegetation period is proposed. Our calculations demonstrate a good correlation between the S(t) value and crop yield (in the range from 0.85 to 0.90); the higher is S(t) for the vegetation period, the higher is the crop yield. S(t) value can be used to calculate the increase in dry and wet biomass for various crops during the whole vegetation period with an error of less than 10–12%. The absolute error of crop yield for 110 cultivars of wheat, oats, and barley during the experimental period was ±3–3.5 quintal/ha with the mean crop yield of 14–38 quintal/ha.     

Rapid Dark Recovery of the Invertebrate Early Receptor Potential

The recovery in the dark of the early receptor potential, as a direct manifestation of the state of the visual pigments, has been studied by intracellular recording in the ventral photoreceptors of Limulus and lateral photoreceptors of Balanus. The recovery is exponential with 1/e time constants of about 80 ms at 24°C for both preparations and 1800 ms at 4°C for Balanus. The 24°C rate extrapolates to total recovery of the pigment within 2 s. The later part of the dark adaptation of the late receptor potential, which may take from seconds to minutes in these preparations, appears thus to be unrelated to the state of the pigment.     

Photosynthetic Oxygen Evolution at Low Water Potential in Leaf Discs Lacking an Epidermis

Land plants encountering low water potentials (low _w) closetheir stomata, restricting CO₂ entry and potentially photosynthesis.To determine the impact of stomatal closure, photosyntheticO₂ evolution was investigated in leaf discs from sunflower (Helianthusannuus L.) plants after removing the lower epidermis at low_w. Wounding was minimal as evidenced by O₂ evolution nearlyas rapid as that in intact discs. O₂ evolution was maximal in1 % CO₂ in the peeled discs and was markedly inhibited when_w was below –1·1 MPa. CO₂ entered readily at all_w, as demonstrated by varying the CO₂ concentration. Resultswere the same whether the epidermis was removed before or afterlow _w was imposed. Due to the lack of an epidermis and readymovement of CO₂ through the mesophyll, the loss in O₂ evolvingactivity was attributed entirely to photosynthetic metabolism.Intact leaf discs showed a similar loss in activity when measuredat a CO₂ concentration of 5 %, which supported maximum O₂ evolutionat low _w. In 1 % CO₂, however, O₂ evolution at low _w was belowthe maximum, presumably because stomatal closure restrictedCO₂ uptake. The inhibition was larger than in peeled discs at_w between –1 and –1·5 MPa but became thesame as in peeled discs at lower _w. Therefore, as photosynthesisbegan to be inhibited by metabolism at low _w, stomatal closureadded to the inhibition. As _w became more negative, the inhibitionbecame entirely metabolic.     

Importance of Photosynthetic Cotyledons for Early Growth of Woody Angiosperms

At various times after seed germination, epigeous cotyledons were excised or treated with DCMU (3-(3,4-dichlorophenyl)-1,1-dimethylurea) to inhibit cotyledon photosynthesis of seedlings of Acer negundo L., Ailanthus altissima (Mill.) Swingle, Eucalyptus globulus Labill., Fraxinus pennsylvanica Marsh., Robinia pseudacacia L., and Ulmus americana L. In all species, DCMU inhibited expansion of cotyledons, elongation of roots, initiation of lateral roots, and expansion of foliage leaves. During the first 10 days after radicle emergence decotylization also variously inhibited growth of plant parts. Photosynthetic rates per cotyledon varied among species in the following order: Robinia pseudacacia > Ailanthus altissima≥Fraxinus pennsylvanica > Ulmus americana. The length of time that cotyledon photosynthesis contributed to growth of axial parts varied widely among species.     

Formation of the Photosynthetic Electron Transport System during the Early Phase of Greening in Barley Leaves

The development of photochemical activity in isolated plastids during the early phase of greening of 5-day-old etiolated barley seedlings was studied and related to the appearance of chlorophyll-protein complexes. Photochemical activities of PSI (DCIPH₂ → MV) and PSII (H₂O → DCIP, DPC → DCIP) appeared at 1 and 1.5 hours after the onset of illumination, respectively. However, PSI + PSII activity (H₂O → MV, H₂O → NADP) appeared at 4 hours. The functional plastoquinone pool was noticed, at the latest, from 4 hours. Chloroplast preparations from seedlings of 1 h of greening showed O₂ uptake upon illumination in the absence of MV (−MV activity). This activity peaked at 2 hours of greening, then fell to zero by 6 hours. In contrast to the −MV activity, MV-Hill activity began to increase at 2 hours. Although PSI activity appeared at 1 hour, it failed to reduce ferredoxin until 2 hours. NADP began to be photoreduced at 4 hours in accordance with the appearance of the ferredoxin:NADP reductase activity. After formation of PSI and PSII, electron transport systems between them and between PSI and NADP developed in coordination with each other. Thus, the whole electron transport from water to NADP began to operate at 4 hours.     

The Gondwana Breakup and the History of the Atlantic and Indian Oceans Unveils Two New Clades for Early Neobatrachian Diversification

The largest anuran diversity belongs to the Neobatrachia, which harbor more than five thousand extant species. Here, we propose a new hypothesis for the historical aspects of the neobatrachian evolution with a formal biogeographical analysis. We selected 12 genes for 144 neobatrachian genera and four archaeobatrachian outgroups and performed a phylogenetic analysis using a maximum likelihood algorithm with the rapid bootstrap test. We also estimated divergence times for major lineages using a relaxed uncorrelated clock method. According to our time scale, the diversification of crown Neobatrachia began around the end of the Early Cretaceous. Our phylogenetic tree suggests that the first split of Neobatrachia is related to the geological events in the Atlantic and Indian Oceans. Hence, we propose names for these clades that indicate this connection, i.e., Atlanticanura and Indianura. The Atlanticanura is composed of three major neobatrachian lineages: Heleophrynidae, Australobatrachia and Nobleobatrachia. On the other hand, the Indianura consists of two major lineages: Sooglossoidea and Ranoides. The biogeographical analysis indicates that many neobatrachian splits occurred as a result of geological events such as the separation between South America and Africa, between India and the Seychelles, and between Australia and South America.     

Marine Ecology of Seabirds in Polar Oceans

Patterns of seabird species' distributions differ between theAntarctic and the Arctic. In the Antarctic, distributions areannular or latitudinal, with strong similarities in speciescomposition of seabird communities in all ocean basins at agiven latitude. In the Arctic, communities are arranged meridionally,and show strong differences between ocean basins and, at a givenlatitude, between sides of ocean basins. These differences betweenthe seabird communi ies in the Northern Hemisphere and the SouthernHemisphere reflect differences in the patterns of flow of majorocean current systems. At smaller spatial scales, in both hemispheresthe species composition of seabird communities is sensitiveto changes in watermass characteristics. The distribution of avian biomass is affected by both physicaland biological features of the ocean. In the Antarctic, muchseabird foraging is over deep water, and withinseason, small-scalepatchiness in prey abundance and availability in ice-free watersis likely to be controlledprimarily by the behavior of the prey,rather than by physical features. Thus, prey availability maybe unpredictable in time and space. In contrast, in the NorthernHemisphere, most seabirdforaging is concentrated over shallowcontinental shelves, where currents interact with bathymetryto produce predictable physical features capable of concentratingprey or making prey more easily harvested by seabirds. Ice cover appears to be the most important physical featurein the Antarctic. An entire community of birds is specializedto use prey taken near the ice edge. These prey consist of avariety of species, some of which are normally found much deeperin the water than the birds takingthem can dive. The open-waterportion of the marginal ice zone is also an important foraginghabitat for Antarctic marine birds. In the Arctic, a food webbased on underice algae is used by marine birds, but few ifany data exist on avian use of the open water segment of themarginal ice zone. Recent simultaneous surveys of birds and their prey indicatethat only rarely does the small-scale abundance of birds matchthat of their prey; correlations between predators and preyaregenerally stronger at larger scales. Evidence is accumulatingin the Antarctic that the largestaggregations of krill may bedisproportionately important to foraging seabirds.     

Photosynthetic Potential and Accumulation of Assimilates in the Developing Chloroembryos of Cyamopsis tetragonoloba (L.) Taub

The photosynthetic potential of leaves and chloroembryos of Cyamopsis tetragonoloba (L.) Taub as measured by ¹⁴C-bicarbonate fixation, Hill activity, and in vivo fluorescence transients is compared. On a chlorophyll basis, dark fixation of NaH¹⁴CO₃ in chloroembryos was 1.5 times higher than that of the leaf, whereas carbon fixation under illumination was threefold higher in the leaf than in the embryos. Rates of O₂ evolution were four times more in embryo than in leaf chloroplasts. Shading of developing fruits on the day of anthesis for 10 days induced a 65% reduction in dry matter accumulation in the etiolated embryos, as compared to the normal green embryos of the same fruit half covered by a transparent Polythene sheet. The reduction in dry weight, size of the embryos, and levels of assimilates after shading the developing fruits may be ascribed to partial autotrophy of the chloroembryos.     

175Toward an Optical Biogeography of the Oceans

Invasions of marine communities by seaweeds are increasing globally. Vectors for introductions are primarily aquaculture and the aquarium trade. Attention to these vectors has been minimal, and few, if any, regulations exist to prevent seaweed introductions. Challenges in preventing, eradicating, and controlling invasive seaweeds will be discussed using the invasion of Caulerpa taxifolia in southern California as a model.     

Electron Transfer in the Photosynthetic Membrane: Influence of PH and Surface Potential on the P-680 Reduction Kinetics

The primary electron donor P-680 of the Photosystem-II reaction center was photoxidized by a short flash given after dark adaptation of photosynthetic membranes in which oxygen evolution was inhibited. The P-680⁺ reduction rate was measured under different conditions of pH and salt concentration by following the recovery of the absorption change at 820 nm. As previously reported for Tris-washed chloroplasts (Conjeaud, H., and P. Mathis, 1980, Biochim. Biophys. Acta, 590:353-359) a fast phase of P-680⁺ reduction slows down as the bulk pH decreases. When salt concentration increases, this fast phase becomes faster for pH above 4.5-5 and slower below. A quantitative interpretation is proposed in which the P-680⁺ reduction kinetics by the secondary electron donor Z are controlled by the local pH. This pH, at the membrane level, can be calculated using the Gouy-Chapman theory. A good fit of the results requires to assume that the surface charge density of the inside of the membrane, near the Photosystem-II reaction center, is positive at low pH values and becomes negative as the pH increases, with a local isoelectric point ~4.8. These results lead us to propose a functional scheme in which a pH-dependent proton release is coupled to the electron transfer between secondary and primary donors of Photosystem-II. The H⁺/e ratio varies from 1 at low pH to 0 at high pH, with a real pK ~6.5 for the protonatable species.     

New Pogonophora from the Atlantic and Pacific Oceans

A study of a collection of Pogonophora, made by the R.V. "Vema" in the Atlantic and Pacific Oceans, has revealed a total of 20 species. One of these, Lamellisabella ivanovi, was already known, the rest appear to be new. Seven species are described in detail, the others being represented only by tubes or insignificant fragments.